Observation of ψ(3686)→nn¯ and improved measurement of ψ(3686)→pp¯

Authors:
  • MAM. Ablikim
    M. Ablikim
  • MAM. N. Achasov
    M. N. Achasov
  • SAS. Ahmed
    S. Ahmed
  • MAM. Albrecht
    M. Albrecht
  • DAD. J. Ambrose
    D. J. Ambrose
  • AAA. Amoroso
    A. Amoroso
  • FAF. F. An
    F. F. An
  • QAQ. An
    Q. An
  • JBJ. Z. Bai
    J. Z. Bai
  • OBO. Bakina
    O. Bakina
  • RFR. Baldini Ferroli
    R. Baldini Ferroli
  • YBY. Ban
    Y. Ban

Abstract
We observe the decay ψ(3686)→nn¯ for the first time and measure ψ(3686)→pp¯ with improved accuracy by using 1.07×108 ψ(3686) events collected with the BESIII detector. The measured branching fractions are B(ψ(3686)→nn¯)=(3.06±0.06±0.14)×10−4 and B(ψ(3686)→pp¯)=(3.05±0.02±0.12)×10−4. Here, the first uncertainties are statistical, and the second ones are systematic. With the hypothesis that the polar angular distributions of the neutron and proton in the center-of-mass system obey 1+αcos2θ, we determine the α parameters to be αnn¯=0.68±0.12±0.11 and αpp¯=1.03±0.06±0.03 for ψ(3686)→nn¯ and ψ(3686)→pp¯, respectively.
Funding Information
  • National Natural Science Foundation of China (11235011, 11335008, 11425524, 11505034, 11575077, 11625523, 11635010, 11775246)
  • Ministry of Science and Technology of the People’s Republic of China (2015DFG02380)
  • Chinese Academy of Sciences (KJCX2-YW-N29, KJCX2-YW-N45, QYZDJ-SSW-SLH003)
  • Deutsche Forschungsgemeinschaft (CRC 1044, FOR 2359)
  • Instituto Nazionale di Fisica Nucleare
  • Koninklijke Nederlandse Akademie van Wetenschappen (530-4CDP03)
  • Vetenskapsrådet
  • U.S. Department of Energy (DE-FG02-05ER41374, DE-SC-0010118, DE-SC-0010504, DE-SC-0012069)
  • Rijksuniversiteit Groningen
  • National Research Foundation of Korea (R32-2008-000-10155-010)
  • National Key Basic Research Program of China (2015CB856700)
  • NSFC and CAS (U1332201, U1532257, U1532258, U1632104)
  • 100 Talents Program of CAS
  • National 1000 Talents Program of China
  • INPAC and Shanghai Key Laboratory for Particle Physics and Cosmology
  • Ministry of Development of Turkey (DPT2006K-120470)
  • National Science and Technology fund
  • Helmholtzzentrum fuer Schwerionenforschung GmbH

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